Estimates of Radiation by Superluminal Neutrinos
arXiv:1201.1322 · doi:10.1103/PhysRevD.85.073007
Abstract
We show that the more energetic superluminal neutrinos with quadratically dispersed superluminalities δ=β^2-1, for β=v/c where v is the neutrino velocity, also lose significant energy to radiation to the ν+e^-+e^+ final state in travelling from CERN to Gran Sasso as has been shown to occur for those with constant superluminality by Cohen and Glashow if indeed δ\simeq 5\times 10^{-5}. In addition, we clarify the dependence of such radiative processes on the size of the superluminality.
6 pages, no figures; text re-arranged for journal purposes; improved references; published version(title changed by Editors)
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